Response of Jupiter's inner magnetosphere to the solar wind derived from extreme ultraviolet monitoring of the Io plasma torus-Reference-Cited by-同舟云学术

Response of Jupiter's inner magnetosphere to the solar wind derived from extreme ultraviolet monitoring of the Io plasma torus

Published:2016-12-20 Issue:24 Volume:43 Page:
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Murakami Go¹^ORCID,Yoshioka Kazuo²³^ORCID,Yamazaki Atsushi¹^ORCID,Tsuchiya Fuminori⁴^ORCID,Kimura Tomoki⁵^ORCID,Tao Chihiro⁶⁷^ORCID,Kita Hajime⁴^ORCID,Kagitani Masato⁴^ORCID,Sakanoi Takeshi⁴^ORCID,Uemizu Kazunori⁸,Kasaba Yasumasa⁹^ORCID,Yoshikawa Ichiro¹⁰^ORCID,Fujimoto Masaki¹¹¹

Affiliation:

1. Institute of Space and Astronautical Science Japan Aerospace Exploration Agency Sagamihara Japan

2. Department of Physics Rikkyo University Tokyo Japan

3. Department of Earth and Planetary Science University of Tokyo Tokyo Japan

4. Planetary Plasma and Atmospheric Research Center Tohoku University Sendai Japan

5. Nishina Center for Accelerator‐Based Science RIKEN Wako Japan

6. Institute de Recherche en Astrophysique et Planétologie Université de Toulouse, CNRS Toulouse France

7. National Institute of Information and Communications Technology Koganei Japan

8. National Astronomical Observatory of Japan Mitaka Japan

9. Department of Geophysics Tohoku University Sendai Japan

10. Department of Complexity Science and Engineering University of Tokyo Chiba Japan

11. Earth‐Life Science Institute Tokyo Institute of Technology Tokyo Japan

Funder

Japan Society for the Promotion of Science

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL071675

Reference45 articles.

1. Weakening of Jupiter's main auroral emission during January 2014

2. Magnetospheric Science Objectives of the Juno Mission

3. Dawn-dusk electric field asymmetry of the Io plasma torus

4. The far-ultraviolet main auroral emission at Jupiter – Part 1: Dawn–dusk brightness asymmetries

5. Jupiter's radiation belts

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